If true, that is the type of answer I am looking for. The 55 light year radius 200 seconds post birth, is also more or less the entire universe we can see now, correct? I had thought of it as the entire universe and that the parts now unobservable were simply the horizons that, while once visible, had slid past view. But I see what you are saying and it sounds to me like the right idea, assuming the universe is infinite.
That's right. Unfortunately, many articles use the word "universe" when they really mean "observable universe". So yes, the 55 ly radius is just the size that the *current observable universe was back then*. The entire universe (meaning, not just the currently observable part, but everything), may well have been infinite, and would still be infinite.
There's a term that cosmologists use called the "scale factor" (denoted by the letter a), which is a measure of the distance between objects at any given time. It's normalized such that, at the present time, a=1.
Consider, at the present time, a galaxy that's 10 billion light years away. Back when the scale factor was 0.5 (several billion years ago), that galaxy was 5 billion light years away. When the scale factor reaches 2 (billions of years from now) it'll be 20 billion light years away. Likewise, a galaxy that's now 2 billion light years away was just 1 billion light years away when the scale factor was 0.5, etc.
[This is ignoring motions of the galaxies themselves relative to the underlying spacetime, which actually aren't all that significant when you're talking about scales that are that big.]
Now, if the universe is infinite, then there are actually galaxies at any arbitrary distance you can imagine, well beyond the limits of the *observable* universe. Let's say you have a galaxy at 100 bajillion (define bajillion however you like

) light years away. When the scale factor was 0.5, it was only 50 bajillion light years away, and so on.
The key here is that you have to envision spacetime as being a giant grid that extends to infinity in every direction. The distances between any two points on the grid are given by some comoving distance between them times the scale factor. The comoving distance never changes, just the scale factor. At the instant of the Big Bang, the scale factor was equal to zero, so if you like, that was the one time when the universe wasn't infinite. The Hubble constant is simply the present day growth rate of the scale factor:
http://en.wikipedia.org/wiki/Scale_factor_(Universe)
Most people don't really get this. The common misconception is that the Big Bang represents some kind of explosion, where the matter is bursting out from a center point into an empty void.
But no, there is no "center" to the universe in which an explosion took place, and there is no "empty" part of the universe that matter is moving into. It's just a big (more or less) homogeneous distribution of matter that's getting less and less dense over time as the spacetime that the matter occupies keeps getting more and more stretched out.
Here is an excellent explanation of this by my fellow former Cornell astro grad student Dave Rothstein:
http://curious.astro.cornell.edu/question.php?number=274